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NASA Ames Astrogram – January/February 2024


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Into the Belly of the Rover: VIPER’s Final Science Instrument Installed

by Rachel Hoover

TRIDENT, designed and developed by engineers at Honeybee Robotics in Altadena, California, is the fourth and final science instrument to be installed into VIPER. NASA engineers have already successfully integrated VIPER’s three other science instruments into the rover. These include: the MSOLO (Mass Spectrometer Observing Lunar Operations), NIRVSS (Near-Infrared Volatiles Spectrometer System), and NSS (Neutron Spectrometer System). 

A team of engineers prepares to integrate TRIDENT – short for The Regolith Ice Drill for Exploring New Terrain – into the belly of NASA’s first robotic Moon rover, VIPER (Volatiles Investigating Polar Exploration Rover). 

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A team of engineers prepares to integrate TRIDENT – short for The Regolith Ice Drill for Exploring New Terrain – into the belly of NASA’s first robotic Moon rover, VIPER – short for the Volatiles Investigating Polar Exploration Rover.
Credit: NASA/Bill Stafford

Shortly after TRIDENT was integrated in the clean room at NASA’s Johnson Space Center in Houston, the team also successfully tested its ability to power on, release the locks that hold the drill in place during launch, extend to its full depth of more than three feet (one meter), perform percussive drilling, and return to its stowed position inside the rover.

TRIDENT will dig up soil from below the lunar surface using a rotary percussive drill – meaning it both spins to cut into the ground and hammers to fragment hard material for more energy-efficient drilling. In addition to being able to measure the strength and compactedness of the lunar soil, the drill also carries a temperature sensor to take readings below the surface. VIPER will launch to the Moon aboard Astrobotic’s Griffin lunar lander on a SpaceX Falcon Heavy rocket as part of NASA’s Commercial Lunar Payload Services initiative. It will reach its destination at Mons Mouton near the Moon’s South Pole. Scientists will work with these four instruments to better understand the origin of water and other resources on the Moon, which could support human exploration as part of NASA’s Artemis campaign.

NASA Unveils the X-59 Supersonic Aircraft

On January 12, in Palmdale, California, the NASA unveiled the X-59, a quiet supersonic aircraft, to the world. The aircraft is the centerpiece of NASA’s Quesst mission, the agency, and Lockheed Martin. Quesst is NASA’s mission to demonstrate how the X-49 can fly supersonic without generating loud sonic booms and then survey what people hear when it flies overhead. Reaction to the quieter sonic “thumps” will be shared with regulators who will then consider writing new sound-based rules to lift the ban on the faster-than-sound flight over land. .

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NASA Quesst’s Mission’s X-59 Supersonic Aircraft.

Members of the Quesst mission team are located at all four NASA field centers, all of which have traditionally been associated with the agency’s historic aeronautical research. The team at Ames has spent many hours working on computational fluid dynamics simulations, wind tunnel testing, systems engineer, and test component manufacturing, helping to shape not just the ingenuity of the aircraft, but the Quesst mission entirely. To learn more about the X-59’s impact on the future of aviation and the tradition of rollout ceremonies at NASA, click here

Nahum Alem Receives Modern Day Technology Leader Award

Nahum Alem received a 2024 Modern-Day Technology Leader Award at the 2024 BEYA STEM DTX Conference in Baltimore, Maryland. This is one of the industry’s most important honors in science, technology, enginering, and math (STEM). Alem was recognized at the Technology Recognition Luncheon featuring Modern-Day Technology Leaders and Science Spectrum Trailblazers on Feb. 16. This year’s theme was, “People, Process, Technology.”

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Nahum Alem with the Black Engineer of the Year Modern Day Technology Leaders Award during the BEYA STEM DTX Conference in Baltimore, Maryland on Feb. 16.

The BEYA STEM DTX Conference recognition program is more critical than ever before. One landmark study projects the number of jobs in science, technology, engineering, and math (STEM) in the United States is set to increase in the coming years. According to the National Science Foundation, underrepresented minorities—Hispanic, Black, and American Indian or Alaska Native individuals—made up a higher share of the skilled technical workforce (32%) in 2021 than of workers who were employed in STEM occupations with at least a bachelor’s degree (16%). The conference highlights the importance of not only celebrating the achievements of STEM leaders and professionals but shifting the narrative towards an action-driven strategy to increase the number of minorities with STEM educations and careers. 

Nahum Alem
Nahum Alem award announcement on the digital sign in front of NASA Ames as one drives into the gate.

According to Tyrone D. Taborn, chairman of the BEYA STEM DTX Conference, “Nahum was selected because he is among an extraordinary group of forward-thinking STEM experts. This year the candidates were the strongest and represented the most diverse collection of executive professionals we have had the pleasure of evaluating. From machine learning to medical breakthroughs, this year’s BEYA STEM awardees stand out as superior authorities in their respective fields.”

For nearly four decades, awards presented at the BEYA STEM Conference have honored excellence in STEM and underscored the serious under-representation of minorities in STEM and at senior levels in all disciplines. For 38 years, employers committed to inclusion have chosen the BEYA STEM Conference to exchange best practices and strategies on how to attract and keep diverse talent in scientific and technical fields. 

The 2024 BEYA STEM DTX Conference hosted multiple award presentation events throughout the conference, where Nahum was recognized in addition to all 2024 award recipients for their significant accomplishments in STEM.

Over the three-day event, the conference provided forums on the retention of diverse talent in STEM, continuous improvement, and networking.

The BEYA STEM Awards is a prestigious recognition platform that celebrates the accomplishments of engineers in the STEM fields. For nearly four decades, BEYA has empowered, mentored, and inspired countless individuals, solidifying its position as a beacon of excellence and innovation. https://www.beya.org

Cast of Broadway’s ‘The Wiz’ “Ease on Down the Road” Visits NASA Ames

Members of the cast and crew of “The Wiz” pose inside the National Full-Scale Aerodynamic Complex 40 by 80 foot wind tunnel at NASA’s Ames Research Center in Silicon Valley.
Members of the cast and crew of “The Wiz” pose inside the National Full-Scale Aerodynamic Complex 40 by 80 foot wind tunnel at NASA’s Ames Research Center in Silicon Valley.
Credit: NASA Ames/Brandon Torres

Members of the cast and crew of Broadway production “The Wiz,” currently on tour at San Francisco’s Golden Gate Theatre, visited NASA Ames on Jan. 29 to learn more about the center’s work in air and space.

The group met with center leadership and members of Ames employee advisory groups and toured the Vertical Motion Simulator (VMS), the National Full-Scale Aerodynamics Complex (NFAC), and observed progress on the Automated Reconfigurable Mission Adaptive Digital Assembly Systems (ARMADAS) robots, which use pre-fabricated modular blocks to build structures autonomously, before following the yellow brick road back “home” to Oz. 

NASA Leader Casey Swails Learns About Wildfire Work at NASA Ames

by Abby Tabor

NASA Deputy Associate Administrator Casey Swails views a demonstration on screen in the Airspace Operations Laboratory at NASA Ames. Researchers presented the diverse, long-running efforts in aeronautics at Ames that have helped lay the foundation for agency work related to wildfire response.

NASA Deputy Associate Administrator Casey Swails
NASA Deputy Associate Administrator Casey Swails

These include a project to help integrate drones into the airspace with Unmanned Aircraft Systems Traffic Management, their application to disaster response with the Scalable Traffic Management for Emergency Response Operations project, and how those informed NASA’s newest effort to make wildfire response more targeted and adaptable, the Advanced Capabilities for Emergency Response Operations project.

Michael Falkowski, program manager for the Applied Sciences Wildland Fire program at NASA Headquarters presented wildfire efforts happening under NASA’s Science Mission Directorate, such as the FireSense project, led out of Ames.

The importance of collaborations within NASA and with partner agencies was also highlighted. Wildfires are complex phenomena and tackling their challenges will require the work of many, for the benefit of all.

NASA Astronomer Sees Power in Community, Works to Build More

by Abby Tabor

Science is often portrayed as a solitary affair, where discoveries are made by lone geniuses toiling in isolation. But Dr. Natasha Batalha, an astronomer at NASA Ames says solving problems with the people around her is one of the best parts of her job.

Dr. Natasha Batalha, an astronomer at NASA’s Ames Research Center in California’s Silicon Valley, says collaborating with her teams is one of the best parts of her job.
Dr. Natasha Batalha, an astronomer at NASA Ames says collaborating with her teams is one of the best parts of her job.

 “Oh, man, working with people is all I do!” said Batalha, whose current research involves using NASA’s James Webb Space Telescope to study exoplanets, planets outside our solar system that orbit other stars.

Batalha’s work explores hot, Jupiter-like exoplanets; smaller, rocky exoplanets more similar to Earth; and brown dwarfs, mysterious objects smaller than a star but huge compared to the biggest planets. A single question has driven her since she was a kid: “Does life exist beyond Earth?”

It’s a lofty question, bigger than any one scientist. And that’s the point.

“I love being part of a larger community,” she said, “We’re working together to try to solve this question that people have been asking for centuries.”

However, the particular joy of belonging wasn’t always present in Batalha’s life.

When she was 10, her family moved from Brazil to the U.S., where she was met with culture shock, pressure to assimilate, and a language barrier. She thinks the latter is partly why she gravitated toward the universal language of math.

Eventually, her interests and strengths took shape around astronomy. When she chose to study physics in college, followed by a dual PhD in astronomy and astrobiology, her parents – who are also scientists – helped fill in for the community she was otherwise lacking.

“In high school, I watched female students drop out of my physics classes,” Batalha said. “The honors physics track in college was devoid of women and people of color. I didn’t feel I had a community in my college classes.”

Her mother, Natalie Batalha, is an astronomer who served as project scientist for NASA’s Kepler space telescope– the mission that taught us there are more planets than stars. Natasha’s father is a LatinX physicist. Both her parents had already faced similar challenges in their careers, and having their example to look at of people who had successfully overcome those barriers helped her push on.  

“I identify as female and LatinX, which are both underrepresented groups in STEM,” she said, “but I also have a ton of privilege because my parents are in the field. That gave me a dual perspective on how powerful community is.”

Dr. Natasha Batalha has been hooked on the search for life beyond Earth since elementary school. UC Santa Cruz, UC Regents
Dr. Natasha Batalha has been hooked on the search for life beyond Earth since elementary school. UC Santa Cruz, UC Regents

Since then, empowering her own science community has been a focus of Batalha’s work.

She builds open-source tools, like computer programs for interpreting data, that are available to all. They help scientists use Webb’s exoplanet data to study what climates they may have, the behavior of clouds in their atmospheres, and the chemistry at work there.

“I saw how limiting closed toolsets could be for the community, when only an ‘inner circle’ had access to them,” Batalha said. “So, I wanted to create new tools that would put everyone on the same footing.”

Batalha herself recently used Webb to explore the skies of exoplanet WASP-39 b, a hot gas giant orbiting a star 700 light-years away. She is part of the team that found carbon dioxide and sulfur dioxide there, marking the first time either was detected in an exoplanet atmosphere. Now, she is turning to the difficult-to-discern characteristics of smaller, cooler planets.

Batalha says she’s exactly where her 6th-grade self imagined she would be. In elementary school, she read a biography of NASA astronaut Sally Ride and was hooked by an idea it contained: that in 20 years the kids reading those words could be the ones pioneering the search for life on Mars.

Today’s youth belong to the Artemis Generation, who will explore farther than people have ever gone before. The Artemis program will send the first woman and first person of color to the lunar surface. Missions over time will build a presence at the Moon to unlock a new era of science and prepare for human missions to Mars and beyond. Along the way, scientists will continue to search for signs of life beyond Earth, an endeavor building on the work of many generations and relying on those in the future to carry on the search. 

“That’s something really rewarding about my work at NASA,” she said. “These questions have been asked throughout human history and, by joining the effort to answer them, you’re taking the baton for a while, before passing it on to someone else.”

Ames Employees Gather for Day of Remembrance Ceremony

by Abby Tabor

On Thursday, Jan. 25, Ames employees gathered for the center’s in-person Day of Remembrance Ceremony in front of N200. Also in attendance were former Center Director Scott Hubbard, and former Deputy Center Director Bill Berry. Every year, we take this important opportunity to honor the memories of those who bravely gave their lives in the pursuit of exploration and discovery and to celebrate their contribution to NASA’s missions. This is a solemn moment to reflect and learn from our history and consider our strong culture of safety as we pursue bold advances in our work here at Ames. 

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NASA Ames employees gather at the flagpole in front of N200 to honor the lives lost in human spaceflight and the 17 fallen crew members from Apollo I, the space shuttles Challenger and Columbia.
Credit: NASA Ames/Don Richey

We honor those lost in test flights, missions, and research throughout our history: the Apollo 1 crew – Virgil “Gus” Grissom, Edward White, and Roger Chaffee – who lost their lives at the start of NASA’s pursuit of landing humans on the moon, on January 27, 1967.  We remember the determination of the Challenger crew, who tragically perished 73 seconds into their flight on January 28, 1986 – Michael J. Smith, Dick Scobee, Ronald McNair, Elison Onizuka, Gregory Jarvis, Judith Resnick, and Christa McAuliffe, the first “teacher in space” who leaves a legacy of STEM education that continues today.  We remember the bravery and inspiration of the crew of Columbia – Rick Husband, William McCool, Michael Anderson, Ilan Ramon, David Brown, Laurel Clark, and Ames’ own Kalpana Chawla, friend and coworker of many here, who we lost during a failed shuttle reentry on February 1, 2003.  We also honor the others who gave their lives pursuing the missions of N-A-C-A and NASA research in aerospace and space exploration, whose commitment and courage leave a lasting legacy across our agency and nation. 

During the ceremony, Scott Hubbard, who served on the Columbia Accident Investigation Board (CAIB), spoke about how the accident changed him and what he learned. When sharing a key takeaway from the CAIB report, Hubbard said, “NASA must be a learning agency, and we can’t shy away from our failures or tragedies. We can’t assign them to history so we must learn from them so that [accidents] never occur.” 

As we work to return humans to the moon, and onto Mars, we must reflect on the importance and value of the work we do here at Ames to help ensure the health and safety of those who risk their lives for exploration and the pursuit of knowledge. One example, after the successful return of the Orion capsule from the Artemis 1 test flight a little over a year ago, we discovered that we needed to learn more about the heat shield and its performance during Earth entry from the Moon. Our aero-thermal-dynamics, thermal protection systems, and other experts, along with our arc jet testing team have worked tirelessly to prepare for the first crewed flight of Artemis 2 coming up in 2025.   

Many in our current workforce were not working at the agency when we experienced these unfortunate losses. But we continue to carry the memory of our fallen colleagues and the lessons we’ve learned through our work today. When we look back on the tragedies of the past, we have an opportunity to apply lessons we’ve learned and continue to enforce a safety culture that encourages every voice to be heard and keeps everyone safe. 

Safety is one of NASA’s core values and there’s a reason why it’s listed as NASA’s first core value. We are committed to sustaining a culture that encourages speaking out and sharing concerns. On or off duty, we have a responsibility to keep safety at the center of our work and daily lives – owning and learning from our mistakes and being open to speaking up about concerns with others – to protect our employees, our community, and ourselves. 

Thank you to all those who were able to join us in this moment of reflection. Please take time to look back on NASA’s history, remember our fallen, and consider your health and safety. We cannot do the work that we do without you and your well-being is important us. Know that we have resources available to support you through things that happen at work and beyond. Our community is strong, and let’s continue to care for one another. 

Thank you to those who helped to put our ceremony together, including Lynda Haines, our communications team, and our protective services professionals who keep us safe and secure each and every day. 

Japan Aerospace Exploration Agency (JAXA) Leader Visits Ames to Discuss Space Science and Spaceflight

by Abby Tabor

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Left to right: Institute of Space and Astronautical Science (ISAS) Management and Integration Department Mr. Nobuhiro Takahashi, Center Director Dr. Eugene Tu, and Vice President and Director General (ISAS) Dr. Hitoshi Kuninaka in the N200 Committee Room following an overview of the history and accomplishments of Ames Research Center.
Credit: NASA Ames/Don Richey

Daniel Andrews, project manager for NASA’s Volatiles Investigating Polar Exploration Rover (VIPER) (left), stands next to a full-scale model of the rover alongside visitors from the Japan Aerospace Exploration Agency (JAXA): Dr. Hitoshi Kuninaka, Vice President of JAXA and Director General of JAXA’s Institute of Space and Astronautical Science (ISAS); Nobuhiro Takahashi of the ISAS Management and Integration Department; and Shintaro Chofuku, a JAXA engineer on detail to NASA’s Ames Research Center in California’s Silicon Valley (right), during a visit to Ames on Feb. 1, 2024. 

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Left to Right: Project Manager of the Volatiles Investigating Polar Exploration Rover (VIPER) Dan Andrews, Vice President and Director General, Institute of Space and Astronautical Science (ISAS) and Japan Aerospace Exploration Agency (JAXA) Dr. Hitoshi Kuninaka, ISAS Management and Integration Department Nobuhiro Takahashi, and Shintaro Chofuku with the VIPER model in the lobby of N232.
Credit: NASA Ames/Don Richey

Following briefings about both agencies’ space science and spaceflight missions, Kuninaka toured several Ames facilities supporting NASA and JAXA’s exploration of the solar system. The heat shield for JAXA’s Hayabusa2 mission, which delivered a sample of an asteroid to Earth in 2020, was tested in the center’s arc jet facility, and a portion of that sample is now being studied by Ames researchers. An upcoming JAXA mission to study the two moons of Mars, called Martian Moons eXploration (MMX), was also tested in the arc jet.

Present and future exploration of the Moon was a focus of the day, including a stop at Ames’ Lunar Imaging Lab following the VIPER briefing.  

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Representatives from the Japan Aerospace Exploration Agency (JAXA) visited Ames on Feb. 1. Here they are seen with the Black Swift S2 UAS in the lobby of N232. Left to right: Vice President and Director General Institute of Space and Astronautical Science (ISAS) and JAXA Dr. Hitoshi Kuninaka; Associate Director for Science and Strategy of the Science Directorate at NASA Ames Ryan Spackman; and ISAS Management and Integration Department Nobuhiro Takahashi.
Credit: NASA Ames/Don Richey

VIPER will be delivered to Mons Mouton near the Moon’s South Pole in late 2024 to map water and other potential resources and explore the characteristics of the lunar environment where NASA plans to send future astronauts as part of the Artemis campaign.

Last month, JAXA’s Smart Lander for Investigating Moon (SLIM) arrived on the lunar surface, after reaching its targeted landing site with great accuracy. The mission aimed to demonstrate accurate lunar landing techniques by a small explorer, to help accelerate study of the Moon and planets using lighter exploration systems.

Japan is a significant partner for NASA and for Ames, specifically,” said Center Director Eugene Tu. “From testing with our teams the X-59 quiet supersonic aircraft design to JAXA’s contributions to Artemis and Gateway, where astronauts on future lunar missions will stay, our work together runs broad and deep. We look forward to many more fruitful collaborations.”

Faces of NASA

Rodney Martin – Deputy Discovery & Systems Health Technical Area Lead at Ames

“[In] everyone’s life, they have a pivotal moment when they ask the question, ‘What am I really doing? What am I here for?’ … I’m reminded of a credo that I came up [with] through the evolution of my engagement of a whole bunch of recreational pursuits [including being a marathoner, ultrarunner, and Ironman triathlete] … as well as my professional pursuits. It’s threefold, and here’s what it is:

“[First,] I’m here because I want to be able to challenge myself, to see how much I can squeeze out of me – whatever that is, whatever ‘me’ is. [For example,] I applied to the astronaut candidate program twice, but I failed to make it to the second round. I figured I’d give a go at throwing my hat in the ring! Like with [an earlier career experience of failing out of] the Navy Nuclear Power Training Program, failure in one domain just means that you have to pick yourself up, dust yourself off, and find a new direction – often pursuing stretch goals that are outside of your comfort zone.

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Dr. Rodney Martin, Deputy Discovery and Systems Health Technical Area Lead, NASA’s Ames Research Center
Credit: NASA Ames/Brandon Torres

“[Second,] I want to serve others. I want to find a way to be of use to others, whether it’s in a structured manner or unstructured manner, whether it’s volunteering or just being a civil servant. I really focus on this service aspect; I did become a supervisor about three years ago, and I really take that role seriously. I really have a service-based leadership philosophy. … That’s why I think [mentoring student interns] represented such a [career] highlight for me, because I felt like I was serving their needs. I was helping to really educate them and [provide] knowledge that I want to … transfer to them, to really inspire that next generation of folks.

“… And the third – which I think NASA fits beautifully – is, ‘How do I build the future? How do I help build the future?’

“So again, it’s challenge, service, and building the future. If I don’t do anything else in my entire life except for those three things, I’m at least getting something right. I might be getting everything else entirely wrong, but I can at least work toward those three things.”

Math, Mentorship, Motherhood: Behind the Scenes with NASA Engineers

by Arezu Sarvestani

Engineering is a huge field with endless applications. From aerospace to ergonomics, engineers play an important role in designing, building, and testing technologies all around us.

We asked three engineers at NASA’s Ames Research Center in California’s Silicon Valley to share their experiences, from early challenges they faced in their careers to the day-to-day of being a working engineer.

Give us a look behind the curtain – what is it like being an engineer at NASA?

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In her early days at NASA, Diana Acosta visited her aeronautics research and development team during her maternity leave and her daughter got her first introduction to flight simulation technology.

Diana Acosta: I remember working on my first simulations. We were developing new aircraft with higher efficiency that could operate in new places, such as shorter runways. My team was putting together control techniques and introducing new algorithms to help pilots fly these new aircraft in a safer way. We were creating models and testing, then changing things and testing again. 

We had a simulator that worked on my laptop, and we had a lab with a pilot seat and controls. Every week, I made it my goal to finish my modeling or controls work and put that into the lab environment so that I could fly the aircraft. Every Friday afternoon, I would fly the aircraft in simulation and try out the changes I’d made to see if we were going in a good direction. We’d later integrate that into the Vertical Motion Simulator at Ames (which was used to train all the original space shuttle pilots) so that we could do a full motion test with a collection of pilots to get feedback. 

When simulation time came around, it was during my maternity leave and my team had to take the project to simulation without me. It’s hard to get out of the house with a newborn, but sometimes I’d come by with my daughter and bring brownies to the team. I have two daughters now, and they’ve both been in simulators since a young age.

Diana Acosta is Chief of the Aerospace Simulation and Development Branch at NASA’s Ames Research Center. She has worked at NASA for 17 years.

What’s a challenge you’ve overcome to become an engineer?

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Savvy Verma (standing) reviews simulation activity with Gus Guerra in the Terminal Tactical Separation Assured Flight Environment at NASA’s Ames Research Center in California’s Silicon Valley.
Credit: NASA Ames/Dominic Hart

Savvy Verma: One of the biggest challenges when I started working was that I was sometimes the only woman in a group of men, and I was also much younger. It was sometimes a challenge to get my voice through, or to be heard. I had mentors who taught me to speak up and say things the way I saw them, and that’s what helped me. A good mentor will back you up and support you when you’re in big meetings or giving presentations. They’ll stand up and corroborate you when you’re right, and that goes a long way toward establishing your credibility. It also helped build my confidence, it made me feel like I was on the right track and not out of line. I had both male and female mentors. The female mentor I had always encouraged me to speak my mind. She said the integrity of the experimental result is more important than trying to change things because someone doesn’t like it or doesn’t want to express it a certain way. 

I have a lot more women coworkers now, things have changed a lot. In my group there are four women and three men. 

Savvy Verma is an aerospace engineer at NASA’s Ames Research Center. She has worked at NASA for 22 years.

Can you become an engineer if you struggle with math in school?

Dorcas Kaweesa
Dorcas Kaweesa

Dorcas Kaweesa: When I introduce myself as an engineer, people always say, “You must be good at math,” and I say, “Oh, I work at it.”

When you want to become an engineer, you must remain adaptable, hardworking, and always willing to learn something new. We’re constantly learning, critically thinking, and problem solving. Most of the time we apply mathematical concepts to the engineering problems we’re solving and not every problem is the same. If you struggle with math, my advice is to maintain the passion for learning, especially learning from your mistakes. It comes down to practicing and challenging yourself to think beyond the immediate struggle. There are so many types of math problems and if you’re not good at one, maybe you’re good at another. Maybe it’s just a hiccup. Also, seek help when you need it, there are instructors and peers out there willing to support you.

Personally, I sought help from my instructors, peers, and mentors, in the math and engineering classes that I found challenging. I also practiced a great deal to improve my problem solving and critical thinking skills. In my current role, I am constantly learning new things based on the task at hand. Learning never ends! If you’re struggling with a math concept, don’t give up. Keep trying, keep accepting the challenge, and keep practicing, you’ll steadily make progress. 

Dorcas Kaweesa is mechanical engineer and structures analyst at NASA’s Ames Research Center. She has worked at NASA for more than two years.

SMA Spotlight: Mission Support Creates Career Satisfaction for Zarchi

Each month, the NASA Safety Center profiles a member of the Safety and Mission Assurance (SMA) community, providing insight into their background and highlighting the ways they contribute to the NASA mission. The SMA workforce is made up of a diverse group of professionals who operate across a range of disciplines to assure the safety of NASA personnel and enhance the success of the agency’s portfolio of programs and projects. In January, Kerry Zarchi, division chief, System Safety and Mission Assurance at NASA Ames earned the SMA spotlight recognition.

Zarchi has worked in her SMA role for nearly three years but has been a member of the NASA family for 18 years. Prior to her SMA duties, Zarchi was a computational analyst and supervisor working on heat shields in Ames’ Entry Systems and Technology division.

Zarchi’s supervisory and engineering background has served her well in her SMA role at Ames, which she describes as a “jack-of-all-trades” facility.

Kerry Zarchi, division chief, System Safety and Mission Assurance at NASA Ames earned the SMA spotlight recognition in January.
Kerry Zarchi, division chief, System Safety and Mission Assurance at NASA Ames earned the SMA spotlight recognition in January.

“I am never bored! Because Ames is small, we kind of do it all,” she said. “We have a lot of ‘do-no-harm’ missions, as well as high-risk missions, and we have a lot of critical facilities here.”

Zarchi’s group supports a varied roster of Ames projects, including Volatiles Investigating Polar Exploration Rover (VIPER), Arc Jet Modernization, HelioSwarm, the creation of a procurement Quality Assurance capability, and facilities like wind tunnels and the Vertical Motion Simulator.

In addition to her supervisory duties, Zarchi is enjoying the long-term work of building new leadership roles within her division to give her staff more opportunities.

 “I want to see them go in the different directions they choose,” she said. “Enabling them in their careers is my proudest achievement.”

Throughout her career in multiple roles and levels of responsibility, Zarchi said the best learning experiences she’s had are failures.

“Any time there’s some kind of adversity or challenge, it requires reflection and homework,” she said.

She advises early career employees to embrace those hard situations and not be afraid to ask questions to expand their skills and knowledge.

“The best way to get understanding is by asking questions and speaking up,” she said. “A vital ability that we all need to have, regardless of our role, is the ability to communicate.”

Zarchi believes the SMA community will continue to see funding challenges as well as requirements tailoring support.

“Reliance on funding from projects is a challenge,” she said. “A lot of thought needs to go into making sure we are maintaining our independence, even though we are charging to projects. There’s also a lot of work to be done codifying the tailoring of SMA support to high-risk projects.”

Throughout these challenges, Zarchi encourages her SMA colleagues to understand just how important their roles are to the NASA community.

“I want SMA to know that they’re crucial to NASA’s mission, even if they don’t hear it often or get that feeling,” she said. “It’s vital that this community stays healthy and supportive of each other. I love how everyone I encounter in SMA is so supportive. I admire that and want to embody that as well.”

Zarchi said that the opportunity to have a direct impact on NASA missions is what made her SMA role most appealing.

“What we do is really important, and I appreciate the gravity of the role,” she said. “We touch nearly everything. I want to help spread the word on the importance of SMA and why people should care about it.”

Robot Team Builds High-Performance Digital Structure for NASA

by Gianine Figliozzi

Greater than the sum of its parts: NASA tests the capability of a system that includes simple robots, structural building blocks, and smart algorithms to build functional, high-performance large-scale structures, ultimately enabling autonomous deep-space infrastructure.

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Research engineer Christine Gregg inspects a Mobile Metamaterial Internal Co-Integrator (MMIC-I) builder robot. These simple robots are part of a hardware and software system NASA researchers are developing to autonomously build and maintain high-performance large space structures comprised of building blocks. MMIC-I works by climbing though the interior space of building blocks and bolting them to the rest of the structure during a build or unbolting during disassembly.
Credit: NASA Ames/Dominic Hart

If they build it, we will go – for the long-term.

Future long-duration and deep-space exploration missions to the Moon, Mars, and beyond will require a way to build large-scale infrastructure, such as solar power stations, communications towers, and habitats for crew. To sustain a long-term presence in deep space, NASA needs the capability to construct and maintain these systems in place, rather than sending large pre-assembled hardware from Earth. 

NASA’s Automated Reconfigurable Mission Adaptive Digital Assembly Systems (ARMADAS) team is developing a hardware and software system to meet that need. The system uses different types of inchworm-like robots that can assemble, repair, and reconfigure structural materials for a variety of large-scale hardware systems in space. The robots can do their jobs in orbit, on the lunar surface, or on other planets – even before humans arrive.

Researchers at NASA’s Ames Research Center in California’s Silicon Valley recently performed a laboratory demonstration of the ARMADAS technology and analyzed the system’s performance. During the tests, three robots worked autonomously as a team to build a meters-scale shelter structure – roughly the size of a shed – using hundreds of building blocks.  The team published their results today in Science Robotics.

Research engineer Taiwo Olatunde, left, and intern Megan Ochalek, right, observe as robots move and assemble composite building blocks into a structure.
Research engineer Taiwo Olatunde, left, and intern Megan Ochalek, right, observe as robots move and assemble composite building blocks into a structure. The robots worked on their own to complete the structure in a little over 100 hours of operations. To facilitate the team’s watchful monitoring of the robots’ performance, the demonstration was split over several weeks of regular working hours.
Credit: NASA Ames/Dominic Hart

“The ground assembly experiment demonstrated crucial parts of the system: the scalability and reliability of the robots, and the performance of structures they build. This type of test is key for maturing the technology for space applications,” said Christine Gregg, ARMADAS chief engineer at NASA Ames.  

The high strength, stiffness, and low mass of the structural product is comparable to today’s highest-performance structures, like long bridges, aircraft wings, and space structures – such as the International Space Station’s trusses. Such performance is a giant leap for the field of robotically reconfigurable structures. 

A Scaling Omnidirectional Lattice Locomoting Explorer (SOLL-E) builder robot c
A Scaling Omnidirectional Lattice Locomoting Explorer (SOLL-E) builder robot carries a soccer ball-sized building block called a voxel – short for volumetric pixel – during a demonstration of NASA’s Automated Reconfigurable Mission Adaptive Digital Assembly Systems (ARMADAS) technology at NASA’s Ames Research Center in Silicon Valley. The voxels are made of strong and lightweight composite materials formed into a shape called a cuboctahedron.
Credit: NASA Ames/Dominic Hart

A Reliable System Relies on Building Blocks

Building blocks are also key to the robotic system autonomy and reliability. 

“Generally, it’s very hard to develop robust autonomous robots that can operate in unstructured environments, like a typical construction site. We turn that problem on its head by making very simple and reliable robots that operate in an extremely structured lattice environment,” said Gregg.  

For the demonstration, the ARMADAS team provided plans for the structure, but they didn’t micromanage the robots’ work. Software algorithms did the job of planning the robots’ tasks. The system practiced the build sequence in simulation before the actual run started. 

While in operation, two robots – stepping inchworm style – walked on the exterior of the structure, moving one soccer ball-sized voxel at a time. One robot fetched the voxels from a supply station and passed them to the second robot that, in turn, placed each voxel on its target location. 

A third robot followed these placements, climbing though the interior space of the voxels and bolting each new voxel to the rest of the structure. 

screenshot-2024-02-29-at-4.50.53-pm.png?
Screenshot from a time-lapse showing robots working autonomously as a team, to assemble a meters-scale shelter structure using hundreds of building blocks during a technology demonstration at NASA’s Ames.
Credit: NASA

“Because the robots align each small step to the structure in what is essentially a 3D grid, simple algorithms with low computation and sensing requirements can achieve high-level autonomy goals. The system builds and error-corrects on its own with no machine vision or external means of measurement,” said Gregg. 

Future work will expand the library of voxel types that the robots work with, to include solar panels, electrical connections, shielding, and more. Each new module type will dramatically expand the possible applications because the robots can mix and match them to meet specific needs and locations. The ARMADAS team is also working on new robot capabilities, such as inspection tools, to ensure that autonomously constructed facilities are safe and sound before astronauts arrive. 

ARMADAS’ technology approach increases what we can do with equipment sent for most deep space exploration missions, and how long we can use them. When a mission completes, robots can disassemble space structures, repurpose the building blocks, and construct designs of the future.

Illustration of an astronaut in a spacesuit standing on the lunar surface near structures being built by small robots.
This artist’s concept shows the autonomous assembly of critical infrastructure needed for a long-duration human presence on the Moon. Here robots are using modular building blocks to construct structures (left, center) that can protect crew, science facilities, or equipment from space radiation and micrometeoroids. Robots are building a large antenna atop a tower (right) as part of a lunar communications network.NASA

In Memoriam

Senior Research Scientist Dr. Andrzej Pohorille Dies

It is with great sadness that we share the news of the passing of our friend and colleague Dr. Andrzej (Andrew) Pohorille, on January 6, 2024.  Andrew was a member of the Exobiology Branch at Ames for more than 27 years.
 

Dr. Andrzej (Andrew) Pohorille
Dr. Andrzej (Andrew) Pohorille

Andrew received his Ph.D. in theoretical physics (with specialty in biophysics) from the University of Warsaw. He did his postdoctoral work with Professor Bernard Pullman at the Institut de Biologie Physico-Chimique in Paris. In 1992, he became a professor of Chemistry and Pharmaceutical Chemistry at the University of California San Francisco, and in 1996 he joined the staff at NASA Ames, where he directed the NASA Center for Computational Astrobiology. In 2000, he received a NASA Group Award for Astrobiology, and in 2002 he was awarded the NASA Exceptional Scientific Achievement Medal. In 2005, he was named Distinguished Lecturer at the Centre for Mathematical Modeling and the National Centre for Space Research in the U.K., and the H. Julian Allen Award at Ames in 2010. Most recently, in December 2023, Andrew was awarded the NASA Exceptional Service Medal for “distinguished service and sustained contributions to NASA’s establishment of Astrobiology as a vibrant, rigorous, and accessible scientific discipline.”

Andrew’s main interests were focused on modeling the origins of life, computer simulations of biomolecular systems, modeling genetic and metabolic networks, and statistical mechanics of condensed phases. He also worked on the development of novel computational methods for parallel and distributed computing. Andrew had worked on developing concepts and designing instruments for microbiology experiments on small satellites and in the lunar environment, and on new ways to organize scientific information.

In recent years, Andrew has served as a co-lead on two large projects: Evolutionary processes that drove the emergence and early distribution of life (EPDEL) and Center for Life Detection Research and Service (CLD/RS). In the latter, his main accomplishment was to lead the design, deployment, and upgrades of the Life Detection Knowledge Base.  Andrew coauthored more than 120 peer-reviewed publications.

The nomination for Andrew’s Exceptional Service Medal included the statement, “Through his wide-ranging technical contributions, tireless community organizing, and one-on-one mentorship of many, he exemplifies the meaning of “exceptional service”. 

Andrew will be truly missed by all of us.

Statistical Summary of Activities of the Protective Service Division’s Security/Law Enforcement and Fire Protection Services Units for Period Ending December 2023

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      How are different land cover types affected by land subsidence on the U.S. Atlantic Coast?
      Jordan DiPrima
      Land subsidence is a frequently overlooked geologic hazard that is caused by natural processes and, more recently, anthropogenic stressors. The goal of this study is to observe subsidence trends and hotspots among land cover types on Virginia’s Eastern Shore and Long Island, New York. This study utilizes interferometric synthetic aperture radar, or InSAR, satellite data from Sentinel-1 to map vertical land motion from 2017 to 2023. Land cover data were sourced from Landsat 8 satellite imagery. Subsidence was mapped within the following land cover types on the Eastern Shore: urban, wetland, cropland, temperate or sub-polar grassland, temperate or sub-polar shrubland, mixed forest, and temperate or subpolar needleleaf forest. These land cover types have mean vertical velocities ranging from -0.2 mm/yr to -5.2 mm/yr. Results suggest that land subsidence is most severe in cropland areas on the Eastern Shore, with a mean vertical velocity of -5.2 mm/yr. In contrast, wetlands display the most subsidence on Long Island with a mean vertical velocity of -2.1 mm/yr. Long Island lacked distinct trends among land cover types and instead showed evidence of subsidence hotspots. These hotspots exist in the following land cover types: temperate or sub-polar grassland, barren lands, wetland, cropland, and temperate or sub-polar broadleaf deciduous forest. Overall, Eastern Shore croplands and Long Island wetlands were determined to be the most susceptible land cover types. These findings highlight regions at risk of sea level rise, flooding, and coastal erosion as a result of subsidence. With further research, we can map subsiding landscapes on a global scale to improve resource allocation and mitigation techniques.

      Isabelle Peterson
      Total Thermokarst Lake Changes on the Seward Peninsula, Alaska: 2016 to 2024
      Isabelle Peterson
      Thermokarst landscapes have and will continue to change as the arctic landscape warms due to climate change. Permafrost underlies much of these arctic landscapes, and as it melts, thermokarst landscapes are left behind. The Seward Peninsula in Alaska has an abundance of these landscapes, and thermokarst lakes are present in the northernmost portion. Several lakes have come and gone, but with increasing climate instability and warming of the area, there is a possibility of more permafrost melting, creating more of these lakes. To capture these changes, Harmonized Landsat Sentinel-2 (HLS) imagery were used to create annual lake maps of the northern portion of the Seward Peninsula from 2016 to 2024. Much of the methodology was informed from Jones et al. (2011); however, their study used eCognition, while the present study used ArcGIS Pro. This caused some differences in results likely due to the differences in software, satellite imagery, and the proposed study area. Lake number changes were observed annually. From this annual change, several 10 to 40 ha lakes disappeared and reappeared within the study period, along with smaller lakes filling in where larger lakes once were. Thermokarst lake drainage is a process described by Jones and Arp (2015) which has devastating geomorphological impacts on the surrounding area, creating large drainage troughs which diminish surrounding permafrost in a quick time frame. To capture these events and overall changes, satellite imagery is essential. This is especially true in remote regions which are hard to reach by foot and require flight missions to be scheduled over the area for aerial photography. However, LVIS and other higher resolution aerial instruments would provide higher accuracy when identifying smaller lakes, as satellite imagery does not accurately capture lakes below 1 ha in the study area. This assertion is made due to conflicting results compared to Jones et al (2011). While the methodologies of this study have been executed manually, Qin, Zhang, and Lu (2023) have proposed the idea of using Sentinel-2 imagery to map thermokarst lakes through automatic methods. While automatization has not yet been perfected, the potential is there and can be used to analyze thermokarst areas effectively. With more satellite imagery, annual, monthly, and potentially daily changes can be captured in favorable months to monitor changing landscapes in arctic regions. Thermokarst lakes have been changing, and monitoring them can help in the process of understanding the changing climate in arctic areas, especially through the lens melting permafrost.

      Emmanelle Cuasay
      Finding Refuge in Climate Crisis: Analyzing the Differences between Refugia and Non-Refugia in the Northern Philippines Using Remote Sensing
      Emmanelle Cuasay
      Refugia are areas that are characterized by stable environmental conditions that can act as a refuge for species as Earth’s climate warms. In this study, fourteen Harmonized Landsat Sentinel-2 images from February 2014 – March 2024 of the northern Philippines region were used. The region of interest is the terrestrial biome by Lake Taal. Normalized Difference Vegetation Index (NDVI) maps were created from all fourteen images to determine the NDVI 25th highest quartiles of the long-term average NDVI images and of a dry and wet year NDVI image. These values were then used to create refugia and non-refugia maps using ArcGIS Pro. Land cover data from Sentinel-2 and a digital elevation model (DEM), using the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), were plotted in ArcGIS Pro to determine the slope and aspect of the area. Global Ecosystems Dynamics Investigation (GEDI) data were used to look at forest height of the study area, and the distribution of forest height, slope, aspect, and elevation were plotted to determine their probability densities in refugia and non-refugia areas. Results of this study show increased biomass in refugia areas. This suggests that conservation practices are crucial to aid in the preservation of biodiversity and biomass within these refugia areas.

      Jayce Crayne
      Site-Based Observations of a Saharan Dust Storm’s Impacts on Evapotranspiration in North-Central Florida
      Jayce Crayne
      Saharan dust storms serve an important role in the western Atlantic’s climate in their contribution to Earth’s radiation budget, modulating sea surface temperatures (SSTs), fertilizing ecosystems, and suppressing cloud and precipitation patterns (Yuan et al., 2020). However, Saharan dust storms are expected to become less frequent in this region as SSTs continue to rise (Yuan et al., 2020). Predicting the climate response to this change requires a keen understanding of how the presence of these storms affect evapotranspiration (ET) and its indicators. This study utilizes site-based observational data from an AmeriFlux tower near Gainesville, FL recorded during a large dust storm in late June 2020. The storm’s progression was documented using satellite imagery from Aqua and Terra and aerosol optical depth (AOD) measurements from an Aerosol Robotic Network (AERONET) station co-located with the AmeriFlux tower. Indicators of ET such as surface air temperature, vapor pressure deficit, photosynthetic photon flux density, and net radiation were analyzed. Findings were compared to modeled ET and latent energy flux reanalysis data provided by the Global Land Data Assimilation System (GLDAS). Both model simulations and on-site observations support that ET decreased during the days dust concentrations were heaviest and for a short time thereafter. Cloud cover data adopted from meteorological aerodrome reports (METARs) provided by an automated surface observing system (ASOS) located in Gainesville showed that clouds were not a major contributor in decreasing ET during the days of heaviest dust. The results of this study show a considerable decrease in ET as a result of dust aerosols. Further research is necessary to determine whether changes in ET due to Saharan dust storms are significant enough to alter climates in the western Atlantic and, if so, what the climate response will be if the frequency of storms decreases.

      Brandon Wilson
      Predicting 2025 and 2028 dNBR and dNDIV for Csarf Smith River Complex / Evaluating the Effects of 2019 California Wildfire Fund
      Brandon Wilson
      Biodiverse regions across California remain vulnerable to harmful wildfires year round. Quantifying and measuring these regions’ wildfire resilience is necessary for understanding where/how to allocate environmental resources. Several ecological wildfire studies have been conducted utilizing artificial intelligence and remote sensing to analyze and predict biodiversity damage across wildfire prone regions, including Northern Algeria and Arkansas, USA. The current case study aims to analyze biodiversity damage from the 2023 Csarf Smith River Complex Fire in Six Rivers National Forest, California and predict the difference in Normalized Burn Ratio (dNBR) and difference in Normalized Difference Vegetation Index (dNDVI) for 2025 and 2028 using remote-sensing-based random forest (RF) regression. Furthermore, to observe, holistically, a practical method California has implemented to address state-wide wildfire damage, the 2019 California Wildfire Fund (AB 1054 and AB 111) was evaluated using the synthetic control method (SCM). For this case study, remote sensing data from the United States Geological Survey (USGS) and NASA (Landsat 9 Satellite C2 L2, TerraClimate and the Land Data Assimilation System) were utilized for processing relevant spectral indexes for the RF. Data from NOAA, Energy Information Agency, International Monetary Fund and Bureau of Economic Analysis were utilized as synthetic control datasets to evaluate the effects of the 2019 California Wildfire Fund. Elevated topography in this study area is susceptible to high severity burn effects, while less elevated topography burns less. This result affected dNBR and dNDVI predictions as elevated areas seemingly did not have strong resilience to rampant burns. This demonstrates a direct correlation to potential lower transpiration rates for elevated areas, warranting further analysis. Results of low variance, post-treatment, between the treated unit and the synthetic control unit, poses concern for the positive effect of the 2019 Wildfire Fund.

      Carrie Hashimoto
      Describing changes in evapotranspiration following the 2020 Creek Fire in the southern Sierra Nevada
      Carrie Hashimoto
      Climatic warming and high tree density have caused larger and more severe wildfires to occur in western United States forests over time. Wildfires affect both the hydrology and ecology of forests via alterations to the water balance (e.g., evapotranspiration, streamflow, infiltration, and more) and could shift vegetation communities and subsequent ecosystem structure and function. This project explores ecological characteristics of a landscape that predict the extent to which the Creek Fire in the southern Sierra Nevada has affected evapotranspiration. Strides in understanding of consequential evapotranspiration changes can create pathways to address emerging forest health challenges posed by similar western fires. For analysis, various remote sensing and modeled data were collected from OpenET, the North American Land Data Assimilation System, TerraClimate, Harmonized LandSat Sentinel-2 data, and the Shuttle Radar Topography Mission. Multiple linear regression and generalized additive models were constructed. Relative change in evapotranspiration served as the response variable. Model covariates included average temperature, total precipitation in the preceding months, average soil moisture, elevation, slope, aspect, northness, latitude, pre-fire normalized difference vegetation index (NDVI), and post-fire change in normalized burn ratio (dNBR). Best subset selection with cross validation demonstrated minimization of cross-validation error with a 7-covariate model. This reduced model yields lower complexity and more interpretability while sustaining an adjusted R2 of 0.626, compared to the full model’s adjusted R2 of 0.663. A reduced generalized additive model (GAM) with interaction terms drawn from the linear model variable selection demonstrated an adjusted R2 of 0.695, indicating a better fit that comes at the cost of reduced interpretability and higher computational requirements than the linear models. The goal of this work is to disentangle environmental indicators of post-fire evapotranspiration change, such that predictive modeling of future wildfire impacts on evapotranspiration can be achieved.


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      Last Updated Nov 22, 2024 Related Terms
      General Explore More
      8 min read SARP East 2024 Ocean Remote Sensing Group
      Article 21 mins ago 10 min read SARP East 2024 Atmospheric Science Group
      Article 21 mins ago 11 min read SARP East 2024 Terrestrial Fluxes Group
      Article 22 mins ago View the full article
    • By NASA
      11 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      Return to 2024 SARP Closeout Faculty Advisors:
      Dr. Lisa Haber, Virginia Commonwealth University
      Dr. Brandon Alveshere, Virginia Commonwealth University
      Dr. Chris Gough, Virginia Commonwealth University
      Graduate Mentor:
      Mindy Priddy, Virginia Commonwealth University

      Mindy Priddy, Graduate Mentor
      Mindy Priddy, graduate mentor for the 2024 SARP Terrestrial Fluxes group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship.

      Angelina De La Torre
      Using NDVI as a Proxy for GPP to Predict Carbon Dioxide Fluxes
      Angelina De La Torre
      Climate change, driven primarily by greenhouse gases, poses a threat to the future of our planet. Among these gases is carbon dioxide (CO₂), which has a much longer atmospheric residence time compared to other greenhouse gases. One potential factor in reducing atmospheric CO₂ enrichment is plant productivity. Gross Primary Productivity (GPP) estimates the amount of CO₂ fixed during photosynthesis. The Normalized Difference Vegetation Index (NDVI) provides insight into the health of an ecosystem by measuring the density and greenness of vegetation. Therefore, it can be inferred that there is a relationship between NDVI and GPP, as greener plants are likely more productive. In this study, we used NDVI as a proxy for GPP and analyzed the effect NDVI had on CO₂ fluxes during California’s wet season between January and March 2023 in a restored tidal freshwater wetland. GPP and CO₂ flux data were obtained from the Dutch Slough AmeriFlux tower in Oakley, California. Landsat data were used to calculate the average NDVI. The influence of NDVI on GPP was assessed using linear regression. A second linear regression was then performed using NDVI and CO₂ flux, of which GPP is one component. We anticipate that wetlands with greater vegetation density will have lower CO₂ emissions.

      Because Landsat data scans in 16-day intervals, daily variation in NDVI could not be observed. This translates to a frequency discrepancy between the Landsat and AmeriFlux data, as AmeriFlux towers measure in half-hour intervals. Additionally, the wet season represented was limited by data availability, as the data before 2023 were unavailable. Despite data limitations in this study, the outlined process could be repeated in various wetland and climate classifications for further analysis of a larger sample size. This study could assist in developing strategies to increase CO₂ sequestration in an attempt to slow the effects of climate change.

      Samarth Jayadev
      Using Machine Learning to Assess Relationships between NDVI and Net Carbon Exchange During the COVID-19 Pandemic
      Samarth Jayadev
      Understanding the movement of carbon between Earth’s land surface and atmosphere is essential for ecosystem monitoring, creating climate change mitigation strategies, and assessing the carbon budget on national to global scales. Measures of greenness serve as indicators of processes such as photosynthesis that control carbon exchange and are vital in modeling of carbon fluxes. NASA’s Orbiting Carbon Observatory (OCO-2) provides high quality measurements of column-averaged CO₂ concentrations that can be used to derive net carbon exchange (NCE), a measure of CO₂ flux between terrestrial ecosystems and the atmosphere.
      From OCO-2, NCE data collected at the land nadir, land glint satellite position combined with in situ sampling can provide accurate measurements on a 1°x1° scale suitable for carbon flux characterization across the contiguous United States (CONUS). Normalized difference vegetation index (NDVI), which ranges from -1 to +1, measures the greenness of vegetation, serving as an indicator of plant density and health. This can help to understand ecosystem to carbon-cycle interactions and be leveraged for determining patterns with NCE. We examined the relationship between NDVI and NCE across CONUS during 2020 using Gradient Boosting Decision Trees (GBDT) which specialize in classifying and predicting non-linear relationships. This algorithm takes multiple weak learners (decision trees) and combines their predictions in an iterative ensemble method to improve prediction accuracy. Feature and permutation importance tests found that January and August (trough and peak NDVI, respectively) were the highest weighted predictor variables related to NCE. The dataset was split in a 90% training 10% test ratio across latitude/longitude grid cells to assess and verify model performance. Using the mean squared error loss function and hyperparameters with optimal estimators, tree depth, sample split, and learning rate the algorithm was able to converge the test predictions to match the deviance of the training data. The gradient boosting model can be applied to different months and years of NDVI/NCE to further explore these relationships or a multitude of research questions. Further studies should consider integrating land use and land cover change variables such as bare land and urbanization to improve predictions of NCE.

      Makai Ogoshi
      Deep-learning Derived Spaceborne Canopy Structural Metrics Predict Forest Carbon Fluxes
      Makai Ogoshi
      Terrestrial and airborne lidar data products describing canopy structure are potent predictors of forest carbon fluxes, but whether satellite data products produce similarly robust indicators of canopy structure is not known. The assessment of contemporary spaceborne lidar and other remote sensing data products as predictors of carbon fluxes is crucial to next generation instrument and data product design and large-spatial scale modeling. We investigated relationships between deciduous broadleaf forest canopy structure, derived from deep-learning models created with lidar data from GEDI and optical imagery from Sentinel-2, and forest carbon exchange. These included comparisons to in-situ continuous net ecosystem exchange (NEE), gross primary production (GPP), and net primary production (NPP). We find that the mean  canopy height from the gridded spaceborne product has a strong correlation with forest NPP, similar to prior analysis with ground-based lidar (portable canopy lidar; PCL). For comparison to NPP, heights taken from the gridded spaceborne product were compared by overlapping the product with nine terrestrial forest sites from the National Ecological Observatory Network (NEON). We used standard deviation of canopy height as a measure of canopy structural complexity. Complexity derived from the gridded spaceborne product does not show the same strong correlation with NPP as found when using PCL. Mean annual GPP and NEE across five years were compared to the gridded spaceborne product at six Fluxnet2015-tower sites with continuous, gap-filled carbon flux data. When compared to in-situ flux tower data, neither mean canopy height nor structural complexity strongly correlate to annual NEE or GPP. Primarily, the finding that derived spaceborne products exhibit a strong correlation between forest canopy height and NPP will advance global-scale application of forest-carbon flux predictions. Secondarily, a variety of limitations highlight shortcomings in the current terrestrial flux data network. A small number of available study sites, both spatially and temporally, and lack of resolution in vertical complexity of canopy structure both contribute to uncertainty in assessing the relationships to NEE and GPP.

      Sebastian Reed
      Porewater Methane Concentrations Vary Significantly Across A Freshwater Tidal Wetland
      Sebastian Reed
      Methane is a potent greenhouse gas that is over 80 times more powerful than CO₂ at trapping heat and accounts for an estimated 30% of global temperature rise associated with climate change. The largest natural source of methane worldwide is wetlands. Despite the role of methane in driving climate change, the magnitude of global annual wetland methane flux remains highly uncertain. This study analyzes the effects of greenness (assessed using Normalized Difference Vegetation Index; NDVI), plant species composition, rooting depth, atmospheric methane concentration, and plant longevity on porewater methane concentration at the Kimages Rice Rivers Center tidal freshwater wetland. Samples for atmospheric and porewater concentrations were conducted in situ in June 2024. For each sampling location (n = 23) we collected whole air samples (WAS) 2m above the marsh surface and porewater samples 5cm below the marsh surface. We visually assessed species composition at each sample location, with 12 species of wetland plants present overall. We used the TRY plant database to find the rooting depth, leaf nitrogen content, and lifespan of each species. Drone multispectral data from 2023 was used to estimate NDVI values. These variables were compared to the pore water methane concentration via stepwise linear regression. Leaf N content, NDVI, plant species, and WAS sampling did not show statistically significant correlation to porewater methane concentration. Rooting depth showed a slight positive correlation with porewater methane (alpha = 0.1, p = 0.08, R^2 = 0.1). Samples with only perennial plants (as opposed to annual plants) had a higher mean value of porewater methane (p = 0.1). Analyzing porewater methane provides insight as to what wetland components affect methanogenesis and methane release, which aids in assessing which plant functional traits are most responsible for driving or mitigating climate change. Results from this study and future research in this area has the potential to more accurately assess how methane cycles through wetlands to the atmosphere.

      Nohemi Rodarte
      Understanding the vertical profile of CO₂ concentration: How carbon dioxide levels change with altitude
      Nohemi Rodarte
      Carbon dioxide (CO₂) is one of the main greenhouse gasses that contribute to global warming.While the relationship between CO₂ concentrations and land cover types, such as forests and urban areas, is well documented, there is limited knowledge of how CO₂ concentrations vary with altitude at fine spatial scales. Guided by our hypothesis that CO₂ levels vary with altitude and increase with elevation, we used airborne data collected from the B200 aircraft, which flew at different altitudes (400 to 1200 feet) above the urban area of Hopewell, Virginia, between 9:40 AM and 10:40 AM. We analyzed the CO₂ concentrations recorded by the flight to obtain the median and range for each 100 feet of altitude. Our results reveal that carbon dioxide concentrations varied significantly across the range of altitudes investigated. Within the area studied, CO₂ concentrations were found to range between 410 and 470 ppm. The distribution of these concentrations along the altitude gradient shows a bimodal pattern, with notable peaks at altitudes of 700 to 800 feet and 1100 to 1200 feet. Although CO₂ levels were present at all measured altitudes, there was a noticeable drop in the mean concentration at 800 feet,which then stabilized until reaching 1,000 feet before rising again. This pattern indicates that the concentrations of this greenhouse gas are not uniformly distributed with altitude, but rather vary significantly, showing higher concentrations at certain elevations and lower concentrations at others. The CO₂ distribution fluctuates with altitude, showing higher or lower levels at specific heights rather than a smooth gradient, indicating that altitude impacts CO₂ concentrations. While we did not identify the drivers of this change, future studies could evaluate how factors such as surface emissions, atmospheric mixing, and local conditions may contribute to vertical CO₂ profiles, since the altitudes we considered in this research are within the troposphere.

      Camille Shaw
      Linking NDVI with CO₂ and CH₄ Fluxes: Insights into Vegetation and Urban Source-Sink Dynamics in the Great Dismal Swamp
      Camille Shaw
      In recent years, carbon dioxide, methane, and other greenhouse gases have gained attention because of their contribution to the rise in Earth’s global mean temperature. Methane and carbon dioxide have various sources and sinks, but an expanding array of sources have created a need to assess ongoing change in carbon balance. This study aims to quantify the relationship between Normalized Difference Vegetation Index, or NDVI, and methane and carbon dioxide fluxes. We measured carbon dioxide and methane concentrations within the boundary layer using the PICARRO instrument, focusing on the Great Dismal Swamp, a forested wetland, and surrounding areas in the Eastern Mid-Atlantic Region. Data collection occurred at various times of day and along different flight paths in 2016, 2017, and 2024, with each year representing data from a single season, either spring or fall, for temporal analysis. We calculated methane and carbon dioxide fluxes along the flight paths using airborne eddy covariance, a method for capturing accurate flux measurements while accounting for the mixing of gases in the boundary layer caused by heat. Additionally, we calculated NDVI for this area using NASA’s Landsat 8 and 9 satellite imagery. Analysis of the afternoon flight data revealed a negative linear correlation between NDVI and carbon dioxide flux. Urban areas, characterized by low NDVI, exhibit a positive carbon dioxide flux as a consequence of emissions from vehicles, while forested areas, with high NDVI, show a negative carbon dioxide flux because of photosynthesis. In contrast, methane flux shows minimal correlation with NDVI. The lack of correlation arises because forested wetlands, with high NDVI, emit substantial amounts of methane, while urban areas, despite having low NDVI, still produce significant methane emissions from landfills and industrial activities. Future research could further investigate how seasonal and diurnal variations influence the correlations between NDVI and greenhouse gases by collecting comprehensive data across all seasons within a given year and at various times of the day.

      Return to 2024 SARP Closeout Share
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      Last Updated Nov 22, 2024 Related Terms
      General Explore More
      8 min read SARP East 2024 Ocean Remote Sensing Group
      Article 21 mins ago 10 min read SARP East 2024 Atmospheric Science Group
      Article 21 mins ago 10 min read SARP East 2024 Hydroecology Group
      Article 21 mins ago View the full article
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